B?rbel Koribalski: Overview (20min.) ... David Barnes: HI total flux comparisons (10min.) ... Martin Zwaan: The HI mass function (20min.) ... Other short contributions and discussions . ... Martin Zwaan: Reliability and Completeness (20min.) ... parameters for the deep catalogue . science from the deep catalogue - who will do what? HI50 meeting: who is presenting what? can the deep catalogue be unveiled at this meeting? ... Martin Meyer: SINGG Project - progress and science projects (20min.) ...

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• Student Contributions for Wildflowers in the Sky
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Next: Discussion Up: No Title Previous: Parameters of binary compact . Under the assumptions made above, we can calculate the binary merging rates in the Galaxy R . ... Figure: The dependence of different compact binary merging rates in a model ``elliptical'' galaxy (where all the stars were formed simultaneously at the moment t =0) with mass M . The horizontal line shows the mean merging rate of binary NS in a spiral galaxy of the same mass with a stationary star formation. ...

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• Discussion
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Next: Chemical abundances Up: HS 0822+3542 - a Previous: H I 21 cm . The main parameters of HS 0822+3542, along with those of the two earlier known local candidate young galaxies, are presented in Table 1 . The distances to all three galaxies for the sake of homogeneity are derived from the radial velocities. ... However, such distance estimates for two galaxies, HS 0822+3542 and I Zw 18 with small radial velocities are rather uncertain. ... The same relates to HS 0822+3542. ...

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• Theory
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Next: About this document Up: Restoration of FOC Imaging Previous: Signal-to-Noise Ratio . In this review I have tried to highlight some of the major factors which must be considered before image restoration work is carried out on FOC data. ... All too frequently, restorations of FOC data are presented in the literature without any substantial discussions of uncertainties or error analysis. ... Before using any image restoration package, take the time to learn 1) What does it do?, ...

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• Ionization and Thermal Structures of the Absorption-Line Systems of Quasars
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... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... Constraints . ... in equation 1 must exceed this value for a source to pass. mindetml . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. minmaskfrac . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. numhexchar . ... 3.5 1.0 1.0 . ...

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• Diagnostic mode
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... -------------- --------------------------------------------------------------- 0845am WELCOME ------- Harvey Tananbaum 0900am A SURVEY of X-RAY SURVEYS ------- MISTs and ANEWs Paul Green 0910am PLENARY SESSION 1: The X-ray Time Machine ----------------- Chair - Georgantopoulos INVITED REVIEW: Amy Barger 25+10 Extragalactic Surveys 0935am 4 CONTRIBUTED ...

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• Topics in AstroStatistics
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• PAUL J. GREEN - Contributing ConcepTests

... Forum: The Linux Kernel Hackers' Guide . Keywords: kernel tuning, file handles, Bus error . ... In a recent comp.os.linux. article I saw a reference to tunable kernel parameters, which I think may help me with a problem I'm having with expireover on a Debian 1.2, Inn 1.4 unoff4 news server. ... I'm runnming 2.0.27, 64mb ram, raid 0 on three 2gb drives for /var/spool/news. ... I've been looking for some docs on tuning kernel parameters like file handles, and can't seem to find it. ...

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. Next: Sub-arrays Up: CHAMELEON Previous: Data base routines Contents . Subsections . Sub-arrays . Bias correction of visibilities . Photometry . Calibration of visibilities . Astrometry data reduction . Introduction . CONSTRICTOR parameters for astrometric reductions . Coherent integration . Dispersion correction . Metrology corrections . A standard recipe . Imaging simulations . Christian Hummel 2015-04-28

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• IAU Symp317 Scientific Program
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... This talk focuses on exploring the connection between Ly absorbers and galaxies. The theorist view of gas in the low z universe is based on the filamentary structures that are evident in simulations based on the CDM paradigm. ... The observer's view of gas in the low-z universe is based on the Ly absorbers which have column densities as low as 10 cm , while galaxies are at column densities of 10 cm . ... The absorber has N cm . ... Can examine LSS defined by gas-rich galaxies around absorbers. ...

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• VLBI at Arecibo Observatory
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... We summarize the discussions that took place during the FITS Birds of a Feather (BoF) session, which was held Monday, September 23, 1996 at 16:00. For completeness we also include a summary of the 1995 FITS BoF, which was never published. ... Oral papers by Clarke, Allen, Mink, Mandel, and Wells were presented in a special FITS afternoon session, and posters were presented by Pence, Farris, Tripicco, and Stobie; see the papers by these authors elsewhere in this volume. ... CFITSIO (Pence) . ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
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• ADASS 2003 Conference Proceedings

seeing -- Create a simulated ground-based star image based on a model of atmospheric turbulence seeing output xdim ydim gamma fwhmx fwhmy . output = "" [image] . The name for the output image to be created. xdim = 512 [integer] . The X dimension for the output image. ydim = 512 [integer] . The Y dimension dor the output image. gamma = 1.6666 [real] . ... For a discussion of the significance of this please see the discussion below and the references given. fwhmx = 5.0 [real] . ...

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• ESLAB 2007
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• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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• Possible manifestation of the gravitational lensing effect in single pulsar
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• VLBI observations of the quasar 3C380

... Status of the numerical solutions and validation 2. ... Coupling of "solid" Earth components, e.g. core ­ mantle (Dehant et al.) ... Consistent relativistic formulation of Earth rotation (Gerlach, Klioner, Soffel) Status of the numerical solutions - 2 · The results from numerical solutions suffer from ­ Simplified solid Earth models ­ Incomplete Earth system models or neglecting of certain parts or neglecting of certain coupling mechanisms ­ Methodological limitations of computations...

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• http://www.gao.spb.ru/english/as/j2014/presentations/ding.pdf
• http://www.gao.spb.ru/russian/psas/ffk2013/part-en.html
• http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf

. N OTE: . Only clusters with R<60 kpc were used to compute the spatial parameters and metallicity gradients for all subsystems except the corona. The numbers in parantheses give the number of clusters for which the corresponding parameter is known. The X O scale length of the old halo is strongly distorted by the observed asymmetry of the distribution of the corresponding clusters projected onto the XY plane ( Fig. 4А ) . discussion in the text | previous table .

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• Vladimir Marsakov Abstracts

... We have observed and studied critical supercurrents, Ic, in cross-type Nb-Cu/Ni-Nb junctions with Josephson layers prepared from diluted ferromagnetic alloys. For suitable values of the exchange energy in the ferromagnet and the F-layer thickness we have observed Ic(T) oscillation with vanishing Ic for the definite values of T and dF. ... Critical supercurrents, Ic, in Nb-Cu(1-x)Ni(x)-Nb Josephson SFS junctions with F-layers prepared from ferromagnetic Cu(1-x)Ni(x) alloys have been studied. ...

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Astronomy Discussion Forums . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums . ... A sk your questions or find answers in the Astronomy Net Forums. ... 3608 posts in 1020 threads, 4:1 ratio . ... Blackholes - Theories, Discussion, etc. 6432 posts in 970 threads, 7:1 ratio . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Halley - Electronic Catalogue Of Comets - an Astronomy Net Software Forum
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V.G. Petukhov . LOW-THRUST TRAJECTORY OPTIMIZATION. ... The optimal control problem is reduced into boundary value problem by means of maximum principle. ... planetary solar and nuclear electric propulsion mission optimization (both rendezvous and flyby) for variable specific impulse problem; . low-thrust trajectory optimization (variable specific impulse problem) within the frame of restricted problem of three bodies, including transfers to the libration points and mission to the Moon; . ...

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... RC0015+0503a . RC0015+0503b . RC0015+0501 . ... Radio source parameters . ... R.A.(B1950) Dec.( ... MHz] size["] flux[mJy] 00:12:48.50 +04:44:53.3 1425.0 10.0x4.6 75 00:12:48.90 +04:44:37.7 7.6x4.6 16 R.A.(J2000) Dec.( J2000) LAS Sp. Morphol. ["] index 00:15:22.62 +05:01:33.6 16.3 1.03 D,FRII 00:15:23.02 +05:01:18.0 ---------------------------------------------- # R.A.(J2000) Dec.( ... R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( ... Last updated 11 Dec 2000 . ...

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